The Ion Chemistry of HNC3O+ C302+ and C30+ in Dense Interstellar Clouds - an Experimental Study

Details The Ion Chemistry of HNC3O+ C302+ and C30+ in Dense Interstellar Clouds - an Experimental Study The Ion Chemistry of HNC3O+ C302+ and C30+ in Dense Interstellar Clouds - an Experimental Study

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.264..862p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 264, NO. 4/OCT15, P. 862, 1993

Astronomy and Astrophysics

Astronomy

1

Molecular Processes - Ism: Clouds - Ism: Molecules

Scientific paper

Interstellar propynal, HCCCHO, may be formed via dissociative recombination of the ion H3C3O+. We report in this work the results of a laboratory investigation, using a selected ion flow tube, of the ion molecule reactions of H3C3O+ (H2CCHCO+), H2C3O+ (H2CCCO+), HC3O+ (HCCCO+), C302+ and C3O+ with a number of neutral reactants relevant to interstellar cloud chemistry. All of the ions HnC3O+ (n = 1-3) are unreactive with hydrogen and should have relatively long cloud lifetimes.

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